All Figures

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f1.ps}\par\end{figure}$ Figure 1: The redshift ( right), and r-band absolute magnitude distributions ( left), for the 91566 galaxies in our sample. The absolute magnitude corresponding to the upper redshift limit (z = 0.095) is M_r=-20.0.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f2.ps}\par\end{figure}$ Figure 2: Left panel: the (u - r) color distribution for all the galaxies in our sample. Central panel: the (u - r) color distribution for galaxies having less than 4 neighbours (corresponding to 10th percentile) compared with the distribution of galaxies having more than 59 neighbours (corresponding to 90th percentile) within 5 Mpc. Right panel: the (u - r) color distribution for galaxies brighter and fainter than M_r = -20.7.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f3.ps}\par\end{figure}$ Figure 3: (u - r) color distribution for galaxies in different environments.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f4.ps}\par\end{figure}$ Figure 4: The trend of $\Delta$ median, defined in the text, as a function of the percentile.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f5.ps}\par\end{figure}$ Figure 5: Top panels: comparison of the color distribution for galaxies having a number of neighbours lesser than the 25th percentile with the color distribution for galaxies having a number of neighbours larger than the 75th percentile. Bottom panels: comparison of the color distribution for galaxies having a number of neighbours lower than the 5th percentile with the color distribution for galaxies having a number of neighbours greater than the 95th percentile. In both panels, the luminosity decreases from left to right.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f6.ps}\par\end{figure}$ Figure 6: (u - r) color distribution for different environment (N is the number of neighbours within 5 Mpc) and for different morphological types.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f7.ps}\par\end{figure}$ Figure 7: (u - r) color distribution for galaxies having different luminosities and different morphological types.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f8.ps}\par\end{figure}$ Figure 8: The (u - r) color distribution for early- and late-type galaxies spectroscopically selected by using the presence of emission lines in the spectra and the FracDev_r and Eclass parameters as in Bernardi et al. (2005). The two distributions are in good agreement.
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In the text

$\begin{figure} \par\includegraphics[width=9cm]{5789f9.ps}\par\end{figure}$ Figure A.1: Top panel: the (u - r) color distribution for a smoothing scale value of 5 Mpc (the reference value), in the underdense and overdense environments. Middle panel: as in the top panel, for three different values of smoothing scale: 2.5 Mpc, 5 Mpc, and 10 Mpc ( left panel: underdense environments; right panel:overdense environments). Bottom panel: differences in the (u - r) color distribution respect to the reference values, for different environments ( left panel: underdense; right panel: overdense).

In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f1.ps}\par\end{figure}$	Figure 1: The redshift ( right), and r-band absolute magnitude distributions ( left), for the 91566 galaxies in our sample. The absolute magnitude corresponding to the upper redshift limit (z = 0.095) is M_r=-20.0.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm]{5789f3.ps}\par\end{figure}$	Figure 3: (u - r) color distribution for galaxies in different environments.
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$\begin{figure} \par\includegraphics[width=8.8cm]{5789f4.ps}\par\end{figure}$	Figure 4: The trend of $\Delta$ median, defined in the text, as a function of the percentile.
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$\begin{figure} \par\includegraphics[width=8.8cm]{5789f6.ps}\par\end{figure}$	Figure 6: (u - r) color distribution for different environment (N is the number of neighbours within 5 Mpc) and for different morphological types.
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$\begin{figure} \par\includegraphics[width=8.8cm]{5789f7.ps}\par\end{figure}$	Figure 7: (u - r) color distribution for galaxies having different luminosities and different morphological types.
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$\begin{figure} \par\includegraphics[width=8.8cm]{5789f8.ps}\par\end{figure}$	Figure 8: The (u - r) color distribution for early- and late-type galaxies spectroscopically selected by using the presence of emission lines in the spectra and the FracDev_r and Eclass parameters as in Bernardi et al. (2005). The two distributions are in good agreement.
Open with DEXTER